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Boosted Three-Dimensional Black-Hole Evolutions with Singularity Excision

Cook, G. B. and Huq, M. F. and Klasky, S. A. and Scheel, M. A. and Abrahams, A. M. and Anderson, A. and Anninos, P. and Baumgarte, T. W. and Bishop, N. T. and Brandt, S. R. and Browne, J. C. and Camarda, K. and Choptuik, M. W. and Correll, R. R. and Evans, C. R. and Finn, L. S. and Fox, G. C. and Gómez, R. and Haupt, T. and Kidder, L. E. and Laguna, P. and Landry, W. and Lehner, L. and Lenaghan, J. and Marsa, R. L. and Masso, J. and Matzner, R. A. and Mitra, S. and Papadopoulos, P. and Parashar, M. and Rezzolla, L. and Rupright, M. E. and Saied, F. and Saylor, P. E. and Seidel, E. and Shapiro, S. L. and Shoemaker, D. and Smarr, L. and Suen, W. M. and Szilágyi, B. and Teukolsky, S. A. and van Putten, M. H. P. M. and Walker, P. and Winicour, J. and York, J. W., Jr. (1998) Boosted Three-Dimensional Black-Hole Evolutions with Singularity Excision. Physical Review Letters, 80 (12). pp. 2512-2516. ISSN 0031-9007. https://resolver.caltech.edu/CaltechAUTHORS:20191009-084004889

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Abstract

Binary black-hole interactions provide potentially the strongest source of gravitational radiation for detectors currently under development. We present some results from the Binary Black Hole Grand Challenge Alliance three-dimensional Cauchy evolution module. These constitute essential steps towards modeling such interactions and predicting gravitational radiation waveforms. We report on single black-hole evolutions and the first successful demonstration of a black hole moving freely through a three-dimensional computational grid via a Cauchy evolution: a hole moving near 6M at 0.1c during a total evolution of duration near 60M.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1103/physrevlett.80.2512DOIArticle
https://arxiv.org/abs/gr-qc/9711078arXivDiscussion Paper
ORCID:
AuthorORCID
Kidder, L. E.0000-0001-5392-7342
Teukolsky, S. A.0000-0001-9765-4526
Additional Information:© 1998 The American Physical Society. Received 26 November 1997. This work was supported by the NSF Binary Black Hole Grand Challenge Grants No. NSF PHY/ASC 93-18152 (ARPA supplemented), No. NSF PHY 93-10083, and Metacenter Grant No. MCA94P015N. Computations were performed at NPAC (Syracuse University), at NCSA (University of Illinois at Urbana-Champaign), and at the Pittsburgh Supercomputing Center.
Funders:
Funding AgencyGrant Number
NSFPHY/ASC 93-18152
NSFPHY 93-10083
MetacenterMCA94P015N
Issue or Number:12
Classification Code:PACS numbers: 04.70.Bw, 04.25.Dm, 04.30.Db
Record Number:CaltechAUTHORS:20191009-084004889
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191009-084004889
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:99177
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:09 Oct 2019 16:15
Last Modified:09 Mar 2020 13:18

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